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There are many ways to derive the
Lorentz transformation In physics, the Lorentz transformations are a six-parameter family of Linear transformation, linear coordinate transformation, transformations from a Frame of Reference, coordinate frame in spacetime to another frame that moves at a constant vel ...
s using a variety of physical principles, ranging from
Maxwell's equations Maxwell's equations, or Maxwell–Heaviside equations, are a set of coupled partial differential equations that, together with the Lorentz force law, form the foundation of classical electromagnetism, classical optics, Electrical network, electr ...
to Einstein's postulates of special relativity, and
mathematical Mathematics is a field of study that discovers and organizes methods, Mathematical theory, theories and theorems that are developed and Mathematical proof, proved for the needs of empirical sciences and mathematics itself. There are many ar ...
tools, spanning from
elementary algebra Elementary algebra, also known as high school algebra or college algebra, encompasses the basic concepts of algebra. It is often contrasted with arithmetic: arithmetic deals with specified numbers, whilst algebra introduces variable (mathematics ...
and
hyperbolic function In mathematics, hyperbolic functions are analogues of the ordinary trigonometric functions, but defined using the hyperbola rather than the circle. Just as the points form a circle with a unit radius, the points form the right half of the ...
s, to
linear algebra Linear algebra is the branch of mathematics concerning linear equations such as :a_1x_1+\cdots +a_nx_n=b, linear maps such as :(x_1, \ldots, x_n) \mapsto a_1x_1+\cdots +a_nx_n, and their representations in vector spaces and through matrix (mathemat ...
and
group theory In abstract algebra, group theory studies the algebraic structures known as group (mathematics), groups. The concept of a group is central to abstract algebra: other well-known algebraic structures, such as ring (mathematics), rings, field ( ...
. This article provides a few of the easier ones to follow in the context of
special relativity In physics, the special theory of relativity, or special relativity for short, is a scientific theory of the relationship between Spacetime, space and time. In Albert Einstein's 1905 paper, Annus Mirabilis papers#Special relativity, "On the Ele ...
, for the simplest case of a Lorentz boost in standard configuration, i.e. two
inertial frame In classical physics and special relativity, an inertial frame of reference (also called an inertial space or a Galilean reference frame) is a frame of reference in which objects exhibit inertia: they remain at rest or in uniform motion relative ...
s moving relative to each other at constant (uniform) relative velocity less than the
speed of light The speed of light in vacuum, commonly denoted , is a universal physical constant exactly equal to ). It is exact because, by international agreement, a metre is defined as the length of the path travelled by light in vacuum during a time i ...
, and using
Cartesian coordinates In geometry, a Cartesian coordinate system (, ) in a plane is a coordinate system that specifies each point uniquely by a pair of real numbers called ''coordinates'', which are the signed distances to the point from two fixed perpendicular o ...
so that the ''x'' and ''x''′ axes are
collinear In geometry, collinearity of a set of Point (geometry), points is the property of their lying on a single Line (geometry), line. A set of points with this property is said to be collinear (sometimes spelled as colinear). In greater generality, t ...
.


Lorentz transformation

In the fundamental branches of
modern physics Modern physics is a branch of physics that developed in the early 20th century and onward or branches greatly influenced by early 20th century physics. Notable branches of modern physics include quantum mechanics, special relativity, and genera ...
, namely
general relativity General relativity, also known as the general theory of relativity, and as Einstein's theory of gravity, is the differential geometry, geometric theory of gravitation published by Albert Einstein in 1915 and is the current description of grav ...
and its widely applicable subset
special relativity In physics, the special theory of relativity, or special relativity for short, is a scientific theory of the relationship between Spacetime, space and time. In Albert Einstein's 1905 paper, Annus Mirabilis papers#Special relativity, "On the Ele ...
, as well as relativistic quantum mechanics and
relativistic quantum field theory In theoretical physics, quantum field theory (QFT) is a theoretical framework that combines field theory and the principle of relativity with ideas behind quantum mechanics. QFT is used in particle physics to construct physical models of suba ...
, the
Lorentz transformation In physics, the Lorentz transformations are a six-parameter family of Linear transformation, linear coordinate transformation, transformations from a Frame of Reference, coordinate frame in spacetime to another frame that moves at a constant vel ...
is the transformation rule under which all
four-vector In special relativity, a four-vector (or 4-vector, sometimes Lorentz vector) is an object with four components, which transform in a specific way under Lorentz transformations. Specifically, a four-vector is an element of a four-dimensional vect ...
s and
tensor In mathematics, a tensor is an algebraic object that describes a multilinear relationship between sets of algebraic objects associated with a vector space. Tensors may map between different objects such as vectors, scalars, and even other ...
s containing
physical quantities A physical quantity (or simply quantity) is a property of a material or system that can be quantified by measurement. A physical quantity can be expressed as a ''value'', which is the algebraic multiplication of a '' numerical value'' and a '' ...
transform from one
frame of reference In physics and astronomy, a frame of reference (or reference frame) is an abstract coordinate system, whose origin (mathematics), origin, orientation (geometry), orientation, and scale (geometry), scale have been specified in physical space. It ...
to another. The prime examples of such four-vectors are the four-position and
four-momentum In special relativity, four-momentum (also called momentum–energy or momenergy) is the generalization of the classical three-dimensional momentum to four-dimensional spacetime. Momentum is a vector in three dimensions; similarly four-momentum i ...
of a
particle In the physical sciences, a particle (or corpuscle in older texts) is a small localized object which can be described by several physical or chemical properties, such as volume, density, or mass. They vary greatly in size or quantity, from s ...
, and for fields the electromagnetic tensor and stress–energy tensor. The fact that these objects transform according to the Lorentz transformation is what mathematically ''defines'' them as vectors and tensors; see
tensor In mathematics, a tensor is an algebraic object that describes a multilinear relationship between sets of algebraic objects associated with a vector space. Tensors may map between different objects such as vectors, scalars, and even other ...
for a definition. Given the components of the four-vectors or tensors in some frame, the "transformation rule" allows one to determine the altered components of the same four-vectors or tensors in another frame, which could be boosted or accelerated, relative to the original frame. A "boost" should not be conflated with spatial translation, rather it's characterized by the relative velocity between frames. The transformation rule itself depends on the relative motion of the frames. In the simplest case of two
inertial frame In classical physics and special relativity, an inertial frame of reference (also called an inertial space or a Galilean reference frame) is a frame of reference in which objects exhibit inertia: they remain at rest or in uniform motion relative ...
s the relative velocity between enters the transformation rule. For
rotating reference frame A rotating frame of reference is a special case of a non-inertial reference frame that is rotation, rotating relative to an inertial reference frame. An everyday example of a rotating reference frame is the surface of the Earth. (This article co ...
s or general non-inertial reference frames, more parameters are needed, including the relative velocity (magnitude and direction), the rotation axis and angle turned through.


Historical background

The usual treatment (e.g.,
Albert Einstein Albert Einstein (14 March 187918 April 1955) was a German-born theoretical physicist who is best known for developing the theory of relativity. Einstein also made important contributions to quantum mechanics. His mass–energy equivalence f ...
's original work) is based on the invariance of the speed of light. However, this is not necessarily the starting point: indeed (as is described, for example, in the second volume of the '' Course of Theoretical Physics'' by
Landau Landau (), officially Landau in der Pfalz (, ), is an autonomous (''kreisfrei'') town surrounded by the Südliche Weinstraße ("Southern Wine Route") district of southern Rhineland-Palatinate, Germany. It is a university town (since 1990), a long ...
and Lifshitz), what is really at stake is the ''locality'' of interactions: one supposes that the influence that one particle, say, exerts on another can not be transmitted instantaneously. Hence, there exists a theoretical maximal speed of information transmission which must be invariant, and it turns out that this speed coincides with the speed of light in vacuum. Newton had himself called the idea of action at a distance philosophically "absurd", and held that gravity had to be transmitted by some agent according to certain laws. Michelson and Morley in 1887 designed an experiment, employing an interferometer and a half-silvered mirror, that was accurate enough to detect aether flow. The mirror system reflected the light back into the interferometer. If there were an aether drift, it would produce a phase shift and a change in the interference that would be detected. However, no phase shift was ever found. The negative outcome of the
Michelson–Morley experiment The Michelson–Morley experiment was an attempt to measure the motion of the Earth relative to the luminiferous aether, a supposed medium permeating space that was thought to be the carrier of light waves. The experiment was performed between ...
left the concept of aether (or its drift) undermined. There was consequent perplexity as to why light evidently behaves like a wave, without any detectable medium through which wave activity might propagate. In a 1964 paper, Erik Christopher Zeeman showed that the causality-preserving property, a condition that is weaker in a mathematical sense than the invariance of the speed of light, is enough to assure that the coordinate transformations are the Lorentz transformations. Norman Goldstein's paper shows a similar result using ''inertiality'' (the preservation of time-like lines) rather than ''causality''.


Physical principles

Einstein based his theory of special relativity on two fundamental postulates. First, all physical laws are the same for all inertial frames of reference, regardless of their relative state of motion; and second, the speed of light in free space is the same in all inertial frames of reference, again, regardless of the relative velocity of each reference frame. The Lorentz transformation is fundamentally a direct consequence of this second postulate.


The second postulate

Assume the second postulate of special relativity stating the constancy of the speed of light, independent of reference frame, and consider a collection of reference systems moving with respect to each other with constant velocity, i.e. inertial systems, each endowed with its own set of
Cartesian coordinates In geometry, a Cartesian coordinate system (, ) in a plane is a coordinate system that specifies each point uniquely by a pair of real numbers called ''coordinates'', which are the signed distances to the point from two fixed perpendicular o ...
labeling the points, i.e. events of spacetime. To express the invariance of the speed of light in mathematical form, fix two events in spacetime, to be recorded in each reference frame. Let the first event be the emission of a light signal, and the second event be it being absorbed. Pick any reference frame in the collection. In its coordinates, the first event will be assigned coordinates x_1, y_1, z_1, ct_1, and the second x_2, y_2, z_2, ct_2. The spatial distance between emission and absorption is \sqrt, but this is also the distance c(t_2-t_1) traveled by the signal. One may therefore set up the equation c^2(t_2 - t_1)^2 - (x_2 - x_1)^2 - (y_2 - y_1)^2 - (z_2 - z_1)^2 = 0. Every other coordinate system will record, in its own coordinates, the same equation. This is the immediate mathematical consequence of the invariance of the speed of light. The quantity on the left is called the '' spacetime interval''. The interval is, for events separated by light signals, the same (zero) in all reference frames, and is therefore called '' invariant''.


Invariance of interval

For the Lorentz transformation to have the physical significance realized by nature, it is crucial that the interval is an invariant measure for ''any'' two events, not just for those separated by light signals. To establish this, one considers an ''infinitesimal'' interval, ds^2 = c^2 dt^2 - dx^2 - dy^2 - dz^2, as recorded in a system K. Let K' be another system assigning the interval ds'^2 to the same two infinitesimally separated events. Since if ds^2 = 0, then the interval will also be zero in any other system (second postulate), and since ds^2 and ds'^2 are infinitesimals of the same order, they must be proportional to each other, ds^2 = a ds'^2. On what may a depend? It may not depend on the positions of the two events in spacetime, because that would violate the postulated ''homogeneity of spacetime''. It might depend on the relative velocity V' between K and K', but only on the speed, not on the direction, because the latter would violate the ''isotropy of space''. Now bring in systems K_1 and K_2, ds^2 = a(V_1)ds_1^2, \quad ds^2 = a(V_2)ds_2^2, \quad ds_1^2 = a(V_)ds_2^2. From these it follows, \frac = a(V_). Now, one observes that on the right-hand side that V_ depend on both V_1 and V_2; as well as on the angle between the ''vectors'' \textbf_1 and \textbf_2. However, one also observes that the left-hand side does not depend on this angle. Thus, the only way for the equation to hold true is if the function a(V) is a constant. Further, by the same equation this constant is unity. Thus, ds^2 = ds'^2 for all systems K'. Since this holds for all infinitesimal intervals, it holds for ''all'' intervals. Most, if not all, derivations of the Lorentz transformations take this for granted. In those derivations, they use the constancy of the speed of light (invariance of light-like separated events) only. This result ensures that the Lorentz transformation is the correct transformation.


Rigorous Statement and Proof of Proportionality of ''ds''2 and ''ds''′2

Theorem: Let n,p\geq 1 be integers, d:= n+p and V a
vector space In mathematics and physics, a vector space (also called a linear space) is a set (mathematics), set whose elements, often called vector (mathematics and physics), ''vectors'', can be added together and multiplied ("scaled") by numbers called sc ...
over \Reals of
dimension In physics and mathematics, the dimension of a mathematical space (or object) is informally defined as the minimum number of coordinates needed to specify any point within it. Thus, a line has a dimension of one (1D) because only one coo ...
d. Let h be an indefinite-inner product on V with
signature A signature (; from , "to sign") is a depiction of someone's name, nickname, or even a simple "X" or other mark that a person writes on documents as a proof of identity and intent. Signatures are often, but not always, Handwriting, handwritt ...
type (n,p). Suppose g is a symmetric bilinear form on V such that the null set of the associated quadratic form of h is contained in that of g (i.e. suppose that for every v \in V, if h(v,v) = 0 then g(v,v)=0). Then, there exists a constant C\in\Reals such that g = Ch . Furthermore, if we assume n\neq p and that g also has signature type (n,p), then we have C>0. Remarks. * In the section above, the term "infinitesimal" in relation to ds^2 is actually referring (pointwise) to a
quadratic form In mathematics, a quadratic form is a polynomial with terms all of degree two (" form" is another name for a homogeneous polynomial). For example, 4x^2 + 2xy - 3y^2 is a quadratic form in the variables and . The coefficients usually belong t ...
over a four-dimensional real vector space (namely the
tangent space In mathematics, the tangent space of a manifold is a generalization of to curves in two-dimensional space and to surfaces in three-dimensional space in higher dimensions. In the context of physics the tangent space to a manifold at a point can be ...
at a point of the spacetime manifold). The argument above is copied almost verbatim from Landau and Lifshitz, where the proportionality of ds^2 and ds'^2 is merely stated as an 'obvious' fact even though the statement is not formulated in a mathematically precise fashion nor proven. This is a non-obvious mathematical fact which needs to be justified; fortunately the proof is relatively simple and it amounts to basic algebraic observations and manipulations. * The above assumptions on h means the following: h:V\times V\to\Reals is a
bilinear form In mathematics, a bilinear form is a bilinear map on a vector space (the elements of which are called '' vectors'') over a field ''K'' (the elements of which are called '' scalars''). In other words, a bilinear form is a function that is linea ...
which is symmetric and non-degenerate, such that there exists an ordered basis \ of V for which h(v_a,v_b) = \begin -1 & \text a = b, \text a,b \in \\\ 1 & \text a = b, \text a,b \in \\\ 0&\text \end An equivalent way of saying this is that h has the matrix representation \begin -I_n & 0 \\0 & I_p\end relative to the ordered basis \. * If we consider the special case where n = 1, p = 3 then we're dealing with the situation of Lorentzian signature in 4-dimensions, which is what relativity is based on (or one could adopt the opposite convention with an overall minus sign; but this clearly doesn't affect the truth of the theorem). Also, in this case, if we assume g and h both have quadratics forms with the same null-set (in physics terminology, we say that g and h give rise to the same light cone) then the theorem tells us that there is a constant C>0 such that g = Ch . Modulo some differences in notation, this is precisely what was used in the section above. Proof of Theorem. Fix a basis \ of V relative to which h has the matrix representation \begin -I_n&0\\ 0&I_p \end . The point is that the vector space V can be decomposed into subspaces V^- (the span of the first n basis vectors) and V^+ (then span of the other p basis vectors) such that each vector in V can be written uniquely as v + w for v \in V^- and w \in V^+; moreover h(v,v) \leq 0, h(w,w) \geq 0 and h(v,w) = 0. So (by bilinearity) h(v+w,v+w) = h(v,v) + h(w,w) Since the first summand on the right in non-positive and the second in non-negative, for any v \in V^- and w \in V^+, we can find a scalar \alpha such that h(v + \alpha w, v + \alpha w) = 0. From now on, always consider v \in V^- and w \in V^+. By bilinearity \begin g(v+w,v+w) &= g(v,v) + g(w,w) + 2g(v,w) \\ g(v-w,v-w) &= g(v,v) + g(w,w) - 2g(v,w) \end If h(v+w,v+w) = 0, then also h(v-w, v-w) = 0 and the same is true for g (since the null-set of h is contained in that of g). In that case, subtracting the two expression above (and dividing by 4) yields 0 = g(v, w) As above, for each v \in V^- and w \in V^+, there is a scalar \alpha such that h(v + \alpha w, v + \alpha w) = 0, so g(v, \alpha w) = 0, which by bilinearity means g(v,w) = 0. Now consider nonzero v, v' \in V^- such that h(v, v) = h(v', v'). We can find w \in V^+ such that 0 = h(v + w, v + w) = h(v,v) + h(w,w) = h(v' + w, v' + w). By the expressions above, g(v,v) = -g(w,w) = g(v', v') Analogically, for w, w' \in V^+, one can show that if h(w,w)=h(w',w'), then also g(w,w)=g(w',w'). So it holds for all vectors in V. For u, u' \in V, if g(u, u) = Ch(u, u) \neq 0, g(u', u') = C'h(u',u') \neq 0 for some C, C' \in \mathbb, we can (scaling one of the if necessary) assume h(u, u) = h(u',u'), which by the above means that C = C'. So g = Ch. Finally, if we assume that g,h both have signature types (n,p) and n\neq p then C >0 (we can't have C = 0 because that would mean g = 0, which is impossible since having signature type (n,p) means it is a non-zero bilinear form. Also, if C<0 , then it means g has n positive diagonal entries and p negative diagonal entries; i.e. it is of signature (p,n)\neq (n,p), since we assumed n\neq p, so this is also not possible. This leaves us with C > 0 as the only option). This completes the proof of the theorem.


Standard configuration

The invariant interval can be seen as a non-positive definite distance function on spacetime. The set of transformations sought must leave this distance invariant. Due to the reference frame's coordinate system's cartesian nature, one concludes that, as in the Euclidean case, the possible transformations are made up of translations and rotations, where a slightly broader meaning should be allowed for the term rotation. The interval is quite trivially invariant under translation. For rotations, there are four coordinates. Hence there are six planes of rotation. Three of those are rotations in spatial planes. The interval is invariant under ordinary rotations too. It remains to find a "rotation" in the three remaining coordinate planes that leaves the interval invariant. Equivalently, to find a way to assign coordinates so that they coincide with the coordinates corresponding to a moving frame. The general problem is to find a transformation such that \begin & c^2(t_2 - t_1)^2 - (x_2 - x_1)^2 - (y_2 - y_1)^2 - (z_2 - z_1)^2 \\ =& c^2(t_2' - t_1')^2 - (x_2' - x_1')^2 - (y_2' - y_1')^2 - (z_2' - z_1')^2. \end To solve the general problem, one may use the knowledge about invariance of the interval of translations and ordinary rotations to assume, without loss of generality, that the frames and are aligned in such a way that their coordinate axes all meet at and that the and axes are permanently aligned and system has speed along the positive . Call this the ''standard configuration''. It reduces the general problem to finding a transformation such that c^2(t_2 - t_1)^2 - (x_2 - x_1)^2 = c^2(t_2' - t_1')^2 - (x_2' - x_1')^2. The standard configuration is used in most examples below. A ''linear'' solution of the simpler problem (ct)^2 - x^2 = (ct')^2 - x'^2 solves the more general problem since coordinate ''differences'' then transform the same way. Linearity is often assumed or argued somehow in the literature when this simpler problem is considered. If the solution to the simpler problem is ''not'' linear, then it doesn't solve the original problem because of the cross terms appearing when expanding the squares.


The solutions

As mentioned, the general problem is solved by translations in spacetime. These do not appear as a solution to the simpler problem posed, while the boosts do (and sometimes rotations depending on angle of attack). Even more solutions exist if one ''only'' insist on invariance of the interval for lightlike separated events. These are nonlinear conformal ("angle preserving") transformations. One has Some equations of physics are conformal invariant, e.g. the
Maxwell's equations Maxwell's equations, or Maxwell–Heaviside equations, are a set of coupled partial differential equations that, together with the Lorentz force law, form the foundation of classical electromagnetism, classical optics, Electrical network, electr ...
in source-free space, but not all. The relevance of the conformal transformations in spacetime is not known at present, but the conformal group in two dimensions is highly relevant in conformal field theory and
statistical mechanics In physics, statistical mechanics is a mathematical framework that applies statistical methods and probability theory to large assemblies of microscopic entities. Sometimes called statistical physics or statistical thermodynamics, its applicati ...
. It is thus the Poincaré group that is singled out by the postulates of special relativity. It is the presence of Lorentz boosts (for which velocity addition is different from mere vector addition that would allow for speeds greater than the speed of light) as opposed to ordinary boosts that separates it from the Galilean group of Galilean relativity. Spatial rotations, spatial and temporal inversions and translations are present in both groups and have the same consequences in both theories (conservation laws of momentum, energy, and angular momentum). Not all accepted theories respect symmetry under the inversions.


Using the geometry of spacetime


Landau & Lifshitz solution

These three hyperbolic function formulae (H1–H3) are referenced below: #\cosh^2\Psi - \sinh^2 \Psi = 1, #\sinh \Psi= \frac, #\cosh\Psi = \frac, The problem posed in standard configuration for a boost in the , where the primed coordinates refer to the ''moving'' system is solved by finding a ''linear'' solution to the simpler problem (ct)^2 - x^2 = (ct')^2 - x'^2. The most general solution is, as can be verified by direct substitution using (H1), To find the role of in the physical setting, record the progression of the origin of , i.e. . The equations become (using first ), x = ct'\sinh \Psi, \quad ct = ct'\cosh \Psi. Now divide: \frac = \tanh \Psi = \frac \Rightarrow \quad \sinh \Psi= \frac, \quad \cosh\Psi = \frac, where was used in the first step, (H2) and (H3) in the second, which, when plugged back in (), gives x=\frac, \quad t= \frac, or, with the usual abbreviations, This calculation is repeated with more detail in section hyperbolic rotation.


Hyperbolic rotation

The Lorentz transformations can also be derived by simple application of the special relativity postulates and using hyperbolic identities. ;Relativity postulates Start from the equations of the spherical wave front of a light pulse, centred at the origin: (ct)^2 - (x^2+y^2+z^2) = (ct')^2 - (x'^2+y'^2+z'^2) =0 which take the same form in both frames because of the special relativity postulates. Next, consider relative motion along the ''x''-axes of each frame, in standard configuration above, so that ''y'' = ''y''′, ''z'' = ''z''′, which simplifies to (ct)^2 - x^2 = (ct')^2 - x'^2 ;Linearity Now assume that the transformations take the linear form: \begin x' & = Ax + Bct \\ ct' & = Cx + Dct \end where ''A'', ''B'', ''C'', ''D'' are to be found. If they were non-linear, they would not take the same form for all observers, since fictitious forces (hence accelerations) would occur in one frame even if the velocity was constant in another, which is inconsistent with inertial frame transformations. Substituting into the previous result: (ct)^2 - x^2 = Cx)^2 + (Dct)^2 + 2CDcxt- Ax)^2 + (Bct)^2 + 2ABcxt and comparing coefficients of , , : \begin - 1 = C^2 - A^2 & \Rightarrow & A^2 - C^2 = 1 \\ c^2 = (Dc)^2 - (Bc)^2 & \Rightarrow & D^2 - B^2 = 1 \\ 2CDc - 2ABc = 0 & \Rightarrow & AB = CD \end ;Hyperbolic rotation: The equations suggest the hyperbolic identity \cosh^2\phi-\sinh^2\phi=1 . Introducing the
rapidity In special relativity, the classical concept of velocity is converted to rapidity to accommodate the limit determined by the speed of light. Velocities must be combined by Einstein's velocity-addition formula. For low speeds, rapidity and velo ...
parameter as a hyperbolic angle allows the consistent identifications A = D = \cosh\phi\,,\quad C = B = -\sinh\phi where the signs after the square roots are chosen so that and increase if and increase, respectively. The hyperbolic transformations have been solved for: \begin x' & = x \cosh\phi - ct \sinh\phi \\ ct' & = -x \sinh\phi + ct \cosh\phi \end If the signs were chosen differently the position and time coordinates would need to be replaced by and/or so that and increase not decrease. To find how relates to the relative velocity, from the standard configuration the origin of the primed frame is measured in the unprimed frame to be (or the equivalent and opposite way round; the origin of the unprimed frame is and in the primed frame it is at ): 0 = vt \cosh\phi - ct \sinh\phi \, \Rightarrow \, \tanh\phi = \frac = \beta and hyperbolic identities \sinh \Psi= \frac,\, \cosh\Psi = \frac leads to the relations between , , and , \cosh\phi = \gamma,\,\quad \sinh\phi=\beta\gamma \,.


From physical principles

The problem is usually restricted to two dimensions by using a velocity along the ''x'' axis such that the ''y'' and ''z'' coordinates do not intervene, as described in standard configuration above.


Time dilation and length contraction

The transformation equations can be derived from
time dilation Time dilation is the difference in elapsed time as measured by two clocks, either because of a relative velocity between them (special relativity), or a difference in gravitational potential between their locations (general relativity). When unsp ...
and
length contraction Length contraction is the phenomenon that a moving object's length is measured to be shorter than its proper length, which is the length as measured in the object's own rest frame. It is also known as Lorentz contraction or Lorentz–FitzGerald ...
, which in turn can be derived from first principles. With and representing the spatial origins of the frames and , and some event , the relation between the position vectors (which here reduce to oriented segments , and ) in both frames is given by: Using coordinates in and in for event M, in frame the segments are , and (since is as measured in ): x = vt + x'/\gamma. Likewise, in frame , the segments are (since is ''as measured in'' ), and : x / \gamma = vt' + x'. By rearranging the first equation, we get x' = \gamma(x - vt), which is the space part of the Lorentz transformation. The second relation gives x = \gamma(x' + vt'), which is the inverse of the space part. Eliminating between the two space part equations gives t' = \gamma t + \frac. that, if \gamma^2=\frac, simplifies to: t' = \gamma(t-vx/c^2), which is the time part of the transformation, the inverse of which is found by a similar elimination of : t = \gamma(t' + vx'/c^2).


Spherical wavefronts of light

The following is similar to that of Einstein. As in the
Galilean transformation In physics, a Galilean transformation is used to transform between the coordinates of two reference frames which differ only by constant relative motion within the constructs of Newtonian physics. These transformations together with spatial rotati ...
, the Lorentz transformation is linear since the relative velocity of the reference frames is constant as a vector; otherwise, inertial forces would appear. They are called inertial or Galilean reference frames. According to relativity no Galilean reference frame is privileged. Another condition is that the speed of light must be independent of the reference frame, in practice of the velocity of the light source. Consider two inertial frames of reference ''O'' and ''O''′, assuming ''O'' to be at rest while ''O''′ is moving with a velocity ''v'' with respect to ''O'' in the positive ''x''-direction. The origins of ''O'' and ''O''′ initially coincide with each other. A light signal is emitted from the common origin and travels as a spherical wave front. Consider a point ''P'' on a spherical
wavefront In physics, the wavefront of a time-varying ''wave field (physics), field'' is the set (locus (mathematics), locus) of all point (geometry), points having the same ''phase (waves), phase''. The term is generally meaningful only for fields that, a ...
at a distance ''r'' and ''r''′ from the origins of ''O'' and ''O''′ respectively. According to the second postulate of the special theory of relativity the
speed of light The speed of light in vacuum, commonly denoted , is a universal physical constant exactly equal to ). It is exact because, by international agreement, a metre is defined as the length of the path travelled by light in vacuum during a time i ...
is the same in both frames, so for the point ''P'': \begin r &= ct \\ r' &= ct'. \end The equation of a sphere in frame ''O'' is given by x^2 + y^2 + z^2 = r^2. For the spherical
wavefront In physics, the wavefront of a time-varying ''wave field (physics), field'' is the set (locus (mathematics), locus) of all point (geometry), points having the same ''phase (waves), phase''. The term is generally meaningful only for fields that, a ...
that becomes x^2 + y^2 + z^2 = (ct)^2. Similarly, the equation of a sphere in frame ''O''′ is given by x'^2 + y'^2 + z'^2 = r'^2, so the spherical wavefront satisfies x'^2 + y'^2 + z'^2 = (ct')^2. The origin ''O''′ is moving along ''x''-axis. Therefore, \begin y' &= y \\ z' &= z. \end must vary linearly with and . Therefore, the transformation has the form x' = \gamma x + \sigma t. For the origin of ''O''′ and are given by \begin x' &= 0 \\ x &= vt, \end so, for all , 0 = \gamma vt + \sigma t and thus \sigma = -\gamma v. This simplifies the transformation to x' = \gamma \left( x - v t \right) where is to be determined. At this point is not necessarily a constant, but is required to reduce to 1 for . The inverse transformation is the same except that the sign of is reversed: x = \gamma \left( x' + v t' \right). The above two equations give the relation between and as: x = \gamma \left \gamma \left( x - v t \right) + v t' \right/math> or t' = \gamma t + \frac. Replacing , , and in the spherical wavefront equation in the ''O''′ frame, x'^2 + y'^2 + z'^2 = (ct')^2, with their expressions in terms of ''x'', ''y'', ''z'' and ''t'' produces: \left( x - v t \right)^2 + y^2 + z^2 = c^2 \left \gamma t + \frac \right2 and therefore, \gamma^2 x^2 + \gamma^2 v^2 t^2 - 2 \gamma^2 v t x + y^2 + z^2 = c^2 t^2 + \frac + 2 \frac which implies, \left - \frac \rightx^2 - 2 v t x + y^2 + z^2 = \left( c^2 - v^2 \right) t^2 + 2 \frac or \left - \frac \rightx^2 - \left 2 v + 2 \frac\rightt x + y^2 + z^2 = \left c^2 - v^2 \rightt^2 Comparing the coefficient of in the above equation with the coefficient of in the spherical wavefront equation for frame ''O'' produces: c^2 - v^2 = c^2 Equivalent expressions for γ can be obtained by matching the ''x''2 coefficients or setting the coefficient to zero. Rearranging: = \frac or, choosing the positive root to ensure that the x and x' axes and the time axes point in the same direction, = \frac which is called the
Lorentz factor The Lorentz factor or Lorentz term (also known as the gamma factor) is a dimensionless quantity expressing how much the measurements of time, length, and other physical properties change for an object while it moves. The expression appears in sev ...
. This produces the Lorentz transformation from the above expression. It is given by \begin x' &= \gamma \left( x - v t \right)\\ t' &= \gamma \left( t - \frac \right) \\ y' &= y \\ z' &= z \end The Lorentz transformation is not the only transformation leaving invariant the shape of spherical waves, as there is a wider set of spherical wave transformations in the context of conformal geometry, leaving invariant the expression \lambda\left(\delta x^2 + \delta y^2 + \delta z^2 - c^2\delta t^2\right). However, scale changing conformal transformations cannot be used to symmetrically describe all laws of nature including
mechanics Mechanics () is the area of physics concerned with the relationships between force, matter, and motion among Physical object, physical objects. Forces applied to objects may result in Displacement (vector), displacements, which are changes of ...
, whereas the Lorentz transformations (the only one implying \lambda = 1) represent a symmetry of all laws of nature and reduce to Galilean transformations at v \ll c.


Galilean and Einstein's relativity


Galilean reference frames

In classical kinematics, the total displacement ''x'' in the R frame is the sum of the relative displacement ''x''′ in frame R′ and of the distance between the two origins ''x'' − ''x''′. If ''v'' is the relative velocity of R′ relative to R, the transformation is: , or . This relationship is linear for a constant , that is when ''R'' and ''R''′ are Galilean frames of reference. In Einstein's relativity, the main difference from Galilean relativity is that space and time coordinates are intertwined, and in different inertial frames ''t'' ≠ ''t''′. Since space is assumed to be homogeneous, the transformation must be linear. The most general linear relationship is obtained with four constant coefficients, ''A'', ''B'', γ, and ''b'': x'=\gamma x + b t t'=A x + B t. The linear transformation becomes the Galilean transformation when γ = ''B'' = 1, ''b'' = −''v'' and ''A'' = 0. An object at rest in the R′ frame at position ''x''′ = 0 moves with constant velocity ''v'' in the R frame. Hence the transformation must yield ''x''′ = 0 if ''x'' = ''vt''. Therefore, ''b'' = −''γv'' and the first equation is written as x'=\gamma \left(x - v t\right) .


Using the principle of relativity

According to the principle of relativity, there is no privileged Galilean frame of reference: therefore the inverse transformation for the position from frame ''R''′ to frame ''R'' should have the same form as the original but with the velocity in the opposite direction, i.o.w. replacing ''v'' with ''-v'': x=\gamma\left(x' - (-v)t'\right), and thus x=\gamma\left(x' + vt'\right) .


Determining the constants of the first equation

Since the speed of light is the same in all frames of reference, for the case of a light signal, the transformation must guarantee that ''t'' = ''x''/''c'' when ''t''′ = ''x''′/''c''. Substituting for ''t'' and ''t''′ in the preceding equations gives: x'= \gamma\left(1 - v/c\right) x , x= \gamma\left(1 + v/c\right) x'. Multiplying these two equations together gives, xx' = \gamma^2 \left(1 - v^2/c^2\right) xx'. At any time after ''t'' = ''t''′ = 0, ''xx''′ is not zero, so dividing both sides of the equation by ''xx''′ results in \gamma=\frac, which is called the "Lorentz factor". When the transformation equations are required to satisfy the light signal equations in the form and ''x''′ = ''ct''′, by substituting the x and x'-values, the same technique produces the same expression for the Lorentz factor.


Determining the constants of the second equation

The transformation equation for time can be easily obtained by considering the special case of a light signal, again satisfying and , by substituting term by term into the earlier obtained equation for the spatial coordinate x'=\gamma (x - v t), \, giving ct'=\gamma \left(ct - \frac x\right), so that t'=\gamma \left(t - \frac x\right), which, when identified with t'=A x + B t, \, determines the transformation coefficients ''A'' and ''B'' as A= -\gamma v/c^2,\, B=\gamma. \, So ''A'' and ''B'' are the unique constant coefficients necessary to preserve the constancy of the speed of light in the primed system of coordinates.


Einstein's popular derivation

In his popular book Einstein derived the Lorentz transformation by arguing that there must be two non-zero coupling constants and such that \begin x' - ct' = \lambda \left( x - ct \right) \\ x' + ct' = \mu \left( x + ct \right) \, \end that correspond to light traveling along the positive and negative x-axis, respectively. For light if and only if . Adding and subtracting the two equations and defining \begin \gamma = \left( \lambda + \mu \right) /2 \\ b = \left( \lambda - \mu \right) /2 ,\, \end gives \begin x' = \gamma x - bct \\ ct' = \gamma ct - bx . \, \end Substituting corresponding to and noting that the relative velocity is , this gives \begin x' = \gamma \left( x - vt \right) \\ t' = \gamma \left( t - \frac x \right) \, \end The constant can be evaluated by demanding as per standard configuration.


Using group theory


From group postulates

Following is a classical derivation (see, e.g.

and references therein) based on group postulates and isotropy of the space. ;Coordinate transformations as a group The coordinate transformations between inertial frames form a Group (mathematics), group (called the proper Lorentz group) with the group operation being the composition of transformations (performing one transformation after another). Indeed, the four group axioms are satisfied: # Closure: the composition of two transformations is a transformation: consider a composition of transformations from the inertial frame ''K'' to inertial frame ''K''′, (denoted as ''K'' → ''K''′), and then from ''K''′ to inertial frame ''K''′′, 'K''′ → ''K''′′ there exists a transformation, 'K'' → ''K''′ 'K''′ → ''K''′′ directly from an inertial frame ''K'' to inertial frame ''K''′′. #
Associativity In mathematics, the associative property is a property of some binary operations that rearranging the parentheses in an expression will not change the result. In propositional logic, associativity is a Validity (logic), valid rule of replaceme ...
: the transformations ( 'K'' → ''K''′ 'K''′ → ''K''′′) 'K''′′ → ''K''′′′and 'K'' → ''K''′( 'K''′ → ''K''′′ 'K''′′ → ''K''′′′) are identical. #
Identity element In mathematics, an identity element or neutral element of a binary operation is an element that leaves unchanged every element when the operation is applied. For example, 0 is an identity element of the addition of real numbers. This concept is use ...
: there is an identity element, a transformation ''K'' → ''K''. #
Inverse element In mathematics, the concept of an inverse element generalises the concepts of opposite () and reciprocal () of numbers. Given an operation denoted here , and an identity element denoted , if , one says that is a left inverse of , and that ...
: for any transformation ''K'' → ''K''′ there exists an inverse transformation ''K''′ → ''K''. ;Transformation matrices consistent with group axioms Consider two inertial frames, ''K'' and ''K''′, the latter moving with velocity with respect to the former. By rotations and shifts we can choose the ''x'' and ''x''′ axes along the relative velocity vector and also that the events and coincide. Since the velocity boost is along the (and ) axes nothing happens to the perpendicular coordinates and we can just omit them for brevity. Now since the transformation we are looking after connects two inertial frames, it has to transform a linear motion in (''t'', ''x'') into a linear motion in coordinates. Therefore, it must be a linear transformation. The general form of a linear transformation is \begin t' \\ x' \end = \begin \gamma & \delta \\ \beta & \alpha \end \begin t \\ x \end, where , , and are some yet unknown functions of the relative velocity . Let us now consider the motion of the origin of the frame ''K''′. In the ''K''′ frame it has coordinates , while in the ''K'' frame it has coordinates . These two points are connected by the transformation \begin t' \\ 0 \end = \begin \gamma & \delta \\ \beta & \alpha \end \begin t \\ vt \end, from which we get \beta = -v\alpha \,. Analogously, considering the motion of the origin of the frame ''K'', we get \begin t' \\ -vt' \end = \begin \gamma & \delta \\ \beta & \alpha \end \begin t \\ 0 \end, from which we get \beta=-v\gamma \,. Combining these two gives and the transformation matrix has simplified, \begin t' \\ x' \end = \begin \gamma & \delta \\ -v\gamma & \gamma \end \begin t \\ x \end. Now consider the group postulate ''inverse element''. There are two ways we can go from the ''K''′ coordinate system to the ''K'' coordinate system. The first is to apply the inverse of the transform matrix to the ''K''′ coordinates: \begin t \\ x \end = \frac \begin \gamma & -\delta \\ v\gamma & \gamma \end \begin t' \\ x' \end. The second is, considering that the ''K''′ coordinate system is moving at a velocity ''v'' relative to the ''K'' coordinate system, the ''K'' coordinate system must be moving at a velocity −''v'' relative to the ''K''′ coordinate system. Replacing ''v'' with −''v'' in the transformation matrix gives: \begin t \\ x \end = \begin \gamma(-v) & \delta(-v) \\ v\gamma(-v) & \gamma(-v) \end \begin t' \\ x' \end, Now the function can not depend upon the direction of because it is apparently the factor which defines the relativistic contraction and time dilation. These two (in an isotropic world of ours) cannot depend upon the direction of . Thus, and comparing the two matrices, we get \gamma^2 + v\delta\gamma = 1. According to the ''closure'' group postulate a composition of two coordinate transformations is also a coordinate transformation, thus the product of two of our matrices should also be a matrix of the same form. Transforming ''K'' to ''K''′ and from ''K''′ to ''K''′′ gives the following transformation matrix to go from ''K'' to ''K''′′: \begin \begin t'' \\ x'' \end & = \begin \gamma(v') & \delta(v') \\ -v'\gamma(v') & \gamma(v') \end \begin \gamma(v) & \delta(v) \\ -v\gamma(v) & \gamma(v) \end \begin t \\ x \end\\ & = \begin \gamma(v')\gamma(v)-v\delta(v')\gamma(v) & \gamma(v')\delta(v)+\delta(v')\gamma(v) \\ -(v'+v)\gamma(v')\gamma(v) & -v'\gamma(v')\delta(v)+\gamma(v')\gamma(v) \end \begin t\\x \end. \end In the original transform matrix, the main diagonal elements are both equal to , hence, for the combined transform matrix above to be of the same form as the original transform matrix, the main diagonal elements must also be equal. Equating these elements and rearranging gives: \begin \gamma(v')\gamma(v)-v\delta(v')\gamma(v) &= -v'\gamma(v')\delta(v)+\gamma(v')\gamma(v) \\ v\delta(v')\gamma(v) &= v'\gamma(v')\delta(v) \\ \frac &= \frac. \end The denominator will be nonzero for nonzero , because is always nonzero; \gamma^2 + v \delta \gamma = 1. If we have the identity matrix which coincides with putting in the matrix we get at the end of this derivation for the other values of , making the final matrix valid for all nonnegative . For the nonzero , this combination of function must be a universal constant, one and the same for all inertial frames. Define this constant as , where has the
dimension In physics and mathematics, the dimension of a mathematical space (or object) is informally defined as the minimum number of coordinates needed to specify any point within it. Thus, a line has a dimension of one (1D) because only one coo ...
of . Solving 1 = \gamma^2 + v\delta\gamma = \gamma^2 (1 + \kappa v^2) we finally get \gamma = 1/\sqrt and thus the transformation matrix, consistent with the group axioms, is given by \begin t' \\ x' \end = \frac \begin 1 & \kappa v \\ -v & 1 \end \begin t \\ x \end. If , then there would be transformations (with ) which transform time into a spatial coordinate and vice versa. We exclude this on physical grounds, because time can only run in the positive direction. Thus two types of transformation matrices are consistent with group postulates: ;Galilean transformations If then we get the Galilean-Newtonian kinematics with the Galilean transformation, \begin t' \\ x' \end = \begin 1 & 0 \\ -v & 1 \end \begin t \\ x \end\;, where time is absolute, , and the relative velocity of two inertial frames is not limited. ;Lorentz transformations If , then we set c = 1/\sqrt which becomes the invariant speed, the speed of light in vacuum. This yields and thus we get special relativity with Lorentz transformation \begin t' \\ x' \end = \frac \begin 1 & \\ -v & 1 \end \begin t \\ x \end\;, where the speed of light is a finite universal constant determining the highest possible relative velocity between inertial frames. If the Galilean transformation is a good approximation to the Lorentz transformation. Only experiment can answer the question which of the two possibilities, or , is realized in our world. The experiments measuring the speed of light, first performed by a Danish physicist Ole Rømer, show that it is finite, and the Michelson–Morley experiment showed that it is an absolute speed, and thus that .


Boost from generators

Using rapidity to parametrize the Lorentz transformation, the boost in the direction is \begin c t' \\ x' \\ y' \\ z' \end = \begin \cosh\phi & -\sinh\phi & 0 & 0\\ -\sinh\phi & \cosh\phi & 0 & 0\\ 0&0&1&0\\ 0&0&0&1\\ \end \begin c\,t \\ x \\ y \\ z \end , likewise for a boost in the -direction \begin c t' \\ x' \\ y' \\ z' \end = \begin \cosh\phi & 0 & -\sinh\phi & 0\\ 0&1&0&0\\ -\sinh\phi &0& \cosh\phi &0\\ 0&0&0&1\\ \end \begin c\,t \\ x \\ y \\ z \end , and the -direction \begin c t' \\ x' \\ y' \\ z' \end = \begin \cosh\phi &0&0&-\sinh\phi\\ 0&1&0&0\\ 0&0&1&0\\ -\sinh\phi&0&0&\cosh\phi\\ \end \begin c\,t \\ x \\ y \\ z \end \,. where are the Cartesian basis vectors, a set of mutually perpendicular unit vectors along their indicated directions. If one frame is boosted with velocity relative to another, it is convenient to introduce a
unit vector In mathematics, a unit vector in a normed vector space is a Vector (mathematics and physics), vector (often a vector (geometry), spatial vector) of Norm (mathematics), length 1. A unit vector is often denoted by a lowercase letter with a circumfle ...
in the direction of relative motion. The general boost is \begin c\,t' \\ x' \\ y' \\ z' \end = \begin \cosh\phi & -n_x\sinh\phi & -n_y\sinh\phi & -n_z\sinh\phi\\ -n_x\sinh\phi & 1+(\cosh\phi-1)n_x^2&(\cosh\phi-1)n_x n_y&(\cosh\phi-1)n_x n_z\\ -n_y\sinh\phi & (\cosh\phi-1)n_y n_x&1+(\cosh\phi-1)n_y^2&(\cosh\phi-1)n_y n_z\\ -n_z\sinh\phi & (\cosh\phi-1)n_z n_x&(\cosh\phi-1)n_z n_y&1+(\cosh\phi-1)n_z^2\\ \end \begin c\,t \\ x \\ y \\ z \end\,. Notice the matrix depends on the direction of the relative motion as well as the rapidity, in all three numbers (two for direction, one for rapidity). We can cast each of the boost matrices in another form as follows. First consider the boost in the direction. The Taylor expansion of the boost matrix about is B(\mathbf_x,\phi)=\sum_^\frac\left.\frac\_ where the derivatives of the matrix with respect to are given by differentiating each entry of the matrix separately, and the notation indicates is set to zero ''after'' the derivatives are evaluated. Expanding to first order gives the ''infinitesimal'' transformation B(\mathbf_x,\phi)=I+\phi\left.\frac\_ = \begin 1 & 0 & 0 & 0\\ 0 & 1 & 0 & 0\\ 0 & 0 & 1 & 0\\ 0 & 0 & 0 & 1 \end-\phi \begin 0 & 1 & 0 & 0\\ 1 & 0 & 0 & 0\\ 0 & 0 & 0 & 0\\ 0 & 0 & 0 & 0 \end which is valid if is small (hence and higher powers are negligible), and can be interpreted as no boost (the first term is the 4×4 identity matrix), followed by a small boost. The matrix K_x=\begin0 & 1 & 0 & 0\\ 1 & 0 & 0 & 0\\ 0 & 0 & 0 & 0\\ 0 & 0 & 0 & 0 \end is the '' generator'' of the boost in the direction, so the infinitesimal boost is B(\mathbf_x,\phi)=I-\phi K_x Now, is small, so dividing by a positive integer gives an even smaller increment of rapidity , and of these infinitesimal boosts will give the original infinitesimal boost with rapidity , B(\mathbf_x,\phi)=\left(I-\frac\right)^N In the limit of an infinite number of infinitely small steps, we obtain the finite boost transformation B(\mathbf_x,\phi)=\lim_\left(I-\frac\right)^=e^ which is the limit definition of the exponential due to
Leonhard Euler Leonhard Euler ( ; ; ; 15 April 170718 September 1783) was a Swiss polymath who was active as a mathematician, physicist, astronomer, logician, geographer, and engineer. He founded the studies of graph theory and topology and made influential ...
, and is now true for any . Repeating the process for the boosts in the and directions obtains the other generators K_y=\begin0 & 0 & 1 & 0\\ 0 & 0 & 0 & 0\\ 1 & 0 & 0 & 0\\ 0 & 0 & 0 & 0 \end\,,\quad K_z=\begin0 & 0 & 0 & 1\\ 0 & 0 & 0 & 0\\ 0 & 0 & 0 & 0\\ 1 & 0 & 0 & 0 \end and the boosts are B(\mathbf_y,\phi)=e^\,,\quad B(\mathbf_z,\phi)=e^\,. For any direction, the infinitesimal transformation is (small and expansion to first order) B(\mathbf,\phi)=I+\phi\left.\frac\_ = \begin 1 & 0 & 0 & 0\\ 0 & 1 & 0 & 0\\ 0 & 0 & 1 & 0\\ 0 & 0 & 0 & 1 \end-\phi\begin0 & n_x & n_y & n_z\\ n_x & 0 & 0 & 0\\ n_y & 0 & 0 & 0\\ n_z & 0 & 0 & 0 \end where \begin0 & n_x & n_y & n_z\\ n_x & 0 & 0 & 0\\ n_y & 0 & 0 & 0\\ n_z & 0 & 0 & 0 \end = n_x K_x + n_y K_y + n_z K_z = \mathbf\cdot\mathbf is the generator of the boost in direction . It is the full boost generator, a vector of matrices , projected into the direction of the boost . The infinitesimal boost is B(\mathbf,\phi)=I-\phi(\mathbf\cdot\mathbf) Then in the limit of an infinite number of infinitely small steps, we obtain the finite boost transformation B(\mathbf,\phi)=\lim_\left(I-\frac\right)^=e^ which is now true for any . Expanding the
matrix exponential In mathematics, the matrix exponential is a matrix function on square matrix, square matrices analogous to the ordinary exponential function. It is used to solve systems of linear differential equations. In the theory of Lie groups, the matrix exp ...
of in its power series e^ = \sum_^\frac(-\phi \mathbf\cdot\mathbf)^n we now need the powers of the generator. The square is (\mathbf\cdot\mathbf)^2=\begin1 & 0 & 0 & 0\\ 0 & n_x^2 & n_x n_y & n_x n_z\\ 0 & n_y n_x & n_y^2 & n_y n_z\\ 0 & n_z n_x & n_z n_y & n_z^2 \end but the cube returns to , and as always the zeroth power is the 4×4 identity, . In general the odd powers are (\mathbf\cdot\mathbf)^n = (\mathbf\cdot\mathbf) while the even powers are (\mathbf\cdot\mathbf)^n = (\mathbf\cdot\mathbf)^2 therefore the explicit form of the boost matrix depends only the generator and its square. Splitting the power series into an odd power series and an even power series, using the odd and even powers of the generator, and the Taylor series of and about obtains a more compact but detailed form of the boost matrix \begin e^& = -\sum_^\frac\phi^n(\mathbf\cdot\mathbf)^n+\sum_^ \frac\phi^n(\mathbf\cdot\mathbf)^n\\ & = - \left phi+\frac+\frac +\cdots \right(\mathbf\cdot\mathbf) + I +\left -1 + 1 + \frac \phi^2+\frac\phi^4 +\frac\phi^6 +\cdots\right\mathbf\cdot\mathbf)^2 \\ & = - \sinh\phi(\mathbf\cdot\mathbf) + I +(-1+\cosh\phi)(\mathbf\cdot\mathbf)^2 \end where is introduced for the even power series to complete the Taylor series for . The boost is similar to
Rodrigues' rotation formula In the theory of three-dimensional rotation, Rodrigues' rotation formula, named after Olinde Rodrigues, is an efficient algorithm for rotating a vector in space, given an axis and angle of rotation. By extension, this can be used to transfo ...
, B(\mathbf,\phi) = e^ = I -\sinh\phi(\mathbf\cdot\mathbf)+(\cosh\phi-1)(\mathbf\cdot\mathbf)^2 \,. Negating the rapidity in the exponential gives the inverse transformation matrix, B(\mathbf,-\phi) = e^ = I +\sinh\phi(\mathbf\cdot\mathbf)+(\cosh\phi-1)(\mathbf\cdot\mathbf)^2 \,. In
quantum mechanics Quantum mechanics is the fundamental physical Scientific theory, theory that describes the behavior of matter and of light; its unusual characteristics typically occur at and below the scale of atoms. Reprinted, Addison-Wesley, 1989, It is ...
, relativistic quantum mechanics, and
quantum field theory In theoretical physics, quantum field theory (QFT) is a theoretical framework that combines Field theory (physics), field theory and the principle of relativity with ideas behind quantum mechanics. QFT is used in particle physics to construct phy ...
, a different convention is used for the boost generators; all of the boost generators are multiplied by a factor of the imaginary unit .


From experiments

Howard Percy Robertson and others showed that the Lorentz transformation can also be derived empirically. In order to achieve this, it's necessary to write down coordinate transformations that include experimentally testable parameters. For instance, let there be given a single "preferred" inertial frame X, Y, Z, T in which the speed of light is constant, isotropic, and independent of the velocity of the source. It is also assumed that Einstein synchronization and synchronization by slow clock transport are equivalent in this frame. Then assume another frame x, y, z, t in relative motion, in which clocks and rods have the same internal constitution as in the preferred frame. The following relations, however, are left undefined: * a(v) differences in time measurements, * b(v) differences in measured longitudinal lengths, * d(v) differences in measured transverse lengths, * \varepsilon(v) depends on the clock synchronization procedure in the moving frame, then the transformation formulas (assumed to be linear) between those frames are given by: \begin t & =a(v)T+\varepsilon(v) x\\ x & =b(v)(X-vT)\\ y & =d(v)Y\\ z & =d(v)Z \end \varepsilon (v) depends on the synchronization convention and is not determined experimentally, it obtains the value -v/c^ by using Einstein synchronization in both frames. The ratio between b(v) and d(v) is determined by the
Michelson–Morley experiment The Michelson–Morley experiment was an attempt to measure the motion of the Earth relative to the luminiferous aether, a supposed medium permeating space that was thought to be the carrier of light waves. The experiment was performed between ...
, the ratio between a(v) and b(v) is determined by the Kennedy–Thorndike experiment, and a(v) alone is determined by the Ives–Stilwell experiment. In this way, they have been determined with great precision to 1/a(v)=b(v)=\gamma and d(v)=1, which converts the above transformation into the Lorentz transformation.


See also

* Lorentz group *
Noether's theorem Noether's theorem states that every continuous symmetry of the action of a physical system with conservative forces has a corresponding conservation law. This is the first of two theorems (see Noether's second theorem) published by the mat ...
* Poincaré group *
Proper time In relativity, proper time (from Latin, meaning ''own time'') along a timelike world line is defined as the time as measured by a clock following that line. The proper time interval between two events on a world line is the change in proper time ...
* Relativistic metric *
Spinor In geometry and physics, spinors (pronounced "spinner" IPA ) are elements of a complex numbers, complex vector space that can be associated with Euclidean space. A spinor transforms linearly when the Euclidean space is subjected to a slight (infi ...


Notes


References

* * *{{citation, last=Weinberg, first=S., year=2002, title=The Quantum Theory of Fields, volume=1, isbn=0-521-55001-7, author-link=Steven Weinberg, publisher=
Cambridge University Press Cambridge University Press was the university press of the University of Cambridge. Granted a letters patent by King Henry VIII in 1534, it was the oldest university press in the world. Cambridge University Press merged with Cambridge Assessme ...
, url-access=registration, url=https://archive.org/details/quantumtheoryoff00stev General relativity Special relativity